{"title":"Estimation, prediction, and forecasting of urban solar brightness: A comprehensive benchmarking of empirical, hybrid AI, and Deep-NARMAX models","authors":"Youness EL Mghouchi , Mihaela Tinca Udristioiu","doi":"10.1016/j.jastp.2026.106761","DOIUrl":null,"url":null,"abstract":"<div><div>Understanding the variability of solar brightness is essential for optimising solar energy systems, improving urban air quality assessments, and enhancing environmental forecasting. The aim of this study is to investigate the influence of meteorological and atmospheric pollutant variables—including temperature, relative humidity, precipitation, wind direction, wind speed, PM<sub>2</sub>.<sub>5</sub>, PM<sub>10</sub>, ozone (O<sub>3</sub>), carbon monoxide (CO), SO<sub>2</sub>, O<sub>3</sub>, NO, NO<sub>2</sub>, NO<sub>x</sub> and others—on incoming solar radiation, using solar brightness as a proxy. A comprehensive dataset spanning five years of hourly observations was analysed. Open-source data from four air quality monitoring stations in Craiova, was provided by the Romanian Environmental Agency. The study followed a five-stage approach. First, data preprocessing was conducted to identify and address anomalies, outliers, and missing values, while trends for solar brightness and other studied variables were analysed. In the second stage, the best global solar radiation (GSR) model among 10 GSR models is selected. In the third stage, correlations between solar brightness and other variables, including data provided by the best GSR model, based on exploratory data analysis, were examined. A deep AI-based hybrid approach was applied in the fourth stage to discover the optimal AI predictive model for solar brightness based on related variables. Finally, a deep NARMAX model was elaborated and applied to model and anticipate next hourly solar brightness in Craiova. A set of statistical metrics was employed to assess the results of the models.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"280 ","pages":"Article 106761"},"PeriodicalIF":1.9000,"publicationDate":"2026-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682626000453","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/2/12 0:00:00","PubModel":"Epub","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Understanding the variability of solar brightness is essential for optimising solar energy systems, improving urban air quality assessments, and enhancing environmental forecasting. The aim of this study is to investigate the influence of meteorological and atmospheric pollutant variables—including temperature, relative humidity, precipitation, wind direction, wind speed, PM2.5, PM10, ozone (O3), carbon monoxide (CO), SO2, O3, NO, NO2, NOx and others—on incoming solar radiation, using solar brightness as a proxy. A comprehensive dataset spanning five years of hourly observations was analysed. Open-source data from four air quality monitoring stations in Craiova, was provided by the Romanian Environmental Agency. The study followed a five-stage approach. First, data preprocessing was conducted to identify and address anomalies, outliers, and missing values, while trends for solar brightness and other studied variables were analysed. In the second stage, the best global solar radiation (GSR) model among 10 GSR models is selected. In the third stage, correlations between solar brightness and other variables, including data provided by the best GSR model, based on exploratory data analysis, were examined. A deep AI-based hybrid approach was applied in the fourth stage to discover the optimal AI predictive model for solar brightness based on related variables. Finally, a deep NARMAX model was elaborated and applied to model and anticipate next hourly solar brightness in Craiova. A set of statistical metrics was employed to assess the results of the models.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.